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Table 3.

Percentages of paired galaxies having w2 − w3 >  2.5 selected according to mass and concentration located in the void interior environment, void walls, and field. Standard errors are included.

Regions log10(M*/Msun)< 9.5 log10(M*/Msun)> 9.5 C <  2.5 C >  2.5
Void interior 90 ± 40% 70 ± 20% 90 ± 30% 50 ± 20%
Void walls 90 ± 20% 60 ± 7% 90 ± 10% 42 ± 7%
Field 87 ± 6% 47 ± 1% 86 ± 3% 30 ± 1%

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